IPs
AE Aqr
FO Aqr
XY Ari
V405 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
YY Dra
PQ Gem
DQ Her
EX Hya
NY Lup
V2400 Oph
GK Per
AO Psc
WX Pyx
V1223 Sgr
V1062 Tau
EI UMa
IGR 00234
IGR 15094
IGR 17303
Swift J0732
RX J0704
RX J1803
RX J2133
SDSS J233325
XSS 00564
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Revninvtsev et al. 2010
- Bibinfo (this paper at ADS)
- Revnivtsev, M., Burenin, R., Bikmaev, I., Kniazev, A., Buckley, D.A.H.,
Pretorius, M.L., Khamitov, I., Ak, T., Eker, Z., Melinikov, S.,
Crawford, S., Pavlinsky, M. 2010, A&A, 513, A63.
- Type
- Observational: Optical Photometry.
- Object(s)
- YY Dra,
V1223 Sgr,
IGR J00234+6141,
XSS J00564+4548,
IGR J15094-6649,
IGR J16500-3307, and
IGR J17195-4100.
- Results
- Aperiodic variability of IPs and IP candidates are studied. The
break in the power spectrum is interpreted to be the Keplerian
frequency of the inner edge of the truncated disk.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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